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    Nitrogen in diamond-free ureilite Allan Hills 78019: Clues to the origin of diamond in ureilites

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    Author
    Rai, V. K.
    Murty, S. V. S.
    Ott, U.
    Issue Date
    2002-01-01
    Keywords
    nitrogen
    chondrites
    noble gases
    isotopic compositions
    urilite diamond
    Allan Hills 78019 (ALH)
    
    Metadata
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    Citation
    Rai, V. K., Murty, S. V. S., & Ott, U. (2002). Nitrogen in diamond‐free ureilite Allan Hills 78019: Clues to the origin of diamond in ureilites. Meteoritics & Planetary Science, 37(8), 1045-1055.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/655548
    DOI
    10.1111/j.1945-5100.2002.tb00876.x
    Additional Links
    https://meteoritical.org/
    Abstract
    Nitrogen and noble gases were measured in a bulk sample and in acid-resistant carbon-rich residues of the ureilite Allan Hills (ALH) 78019 which has experienced low shock and is free of diamond. A small amount of amorphous carbon combusting at less than or equal to 500 degrees C carries most of the noble gases, while the major carbon phase consisting of large crystals of graphite combusts at greater than or equal to 800 degrees C, and is almost noble-gas free. Nitrogen on the other hand is present in both amorphous carbon and graphite, with different 15N signatures of -21 ppm and +19 ppm, respectively, distinctly different from the very light nitrogen (about -100 ppm) of ureilite diamond. Amorphous carbon in ALH 78019 behaves similar to phase Q of chondrites with respect to noble gas release pattern, behavior towards oxidizing acids as well as nitrogen isotopic composition. In situ conversion of amorphous carbon or graphite to diamond through shock would require an isotopic fractionation of 8 to 12% for nitrogen favoring the light isotope, an unlikely proposition, posing a severe problem for the widely accepted shock origin of ureilite diamond.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2002.tb00876.x
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    Meteoritics & Planetary Science, Volume 37, Number 8 (2002)

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